High radiation detection performance from photoactive semiconductor single crystals

ABSTRACT

Methods and devices for detecting incident radiation are provided. The methods and devices use high quality single-crystals of photoactive semiconductor compounds in combination with metal anodes and metal cathodes that provide for enhanced photodetector performance.

CROSS-REFERENCE TO RELATED APPLICATIONS

This application is a National Stage of International Application No. PCT/US2018/049708, filed Sep. 6, 2018, which claims the benefit of U.S. Patent Application No. 62/555,248, filed Sep. 7, 2017, the contents of which are herein incorporated by reference.

REFERENCE TO GOVERNMENT RIGHTS

This invention was made with government support under 2014-DN-077-ARI086-01 awarded by the Department of Homeland Security. The government has certain rights in the invention.

BACKGROUND

The demand for high performance radiation detectors based on compound semiconductors is high, owing to their broad potential applications in the fields of homeland security, industrial and medical imaging, and fundamental scientific research. Previously developed materials have remained in use for decades, as the search for low-cost, promising compounds with desirable properties, such as high density, high atomic number (Z), suitable bandgap (E_(g)), high electrical resistivity (ρ) and high mobility-lifetime (μτ) product, has continued. To ensure sufficient charge collection efficiency (CCE) and high resolution of the energy resolved spectrum, the mean free path (μτE) of the materials should be much larger than the thickness of the device under a certain electrical field E. This means the charge carriers must move through the detector volume unimpeded, and also implies the need for extremely low concentrations of electrically-active and carrier-trapping defects.

Because high performance radiation detectors require such specific, correlated properties, only a few conventional compounds (binary chalcogenides and halides) have been found that have demonstrated an encouraging spectroscopic response. In addition, only a few compounds have been developed with a view toward commercial applications, due to the difficulties or high cost in obtaining high-quality, reproducible, single crystals. Among these, CdTe and CdTe-related pseudo-binary compounds (such as CdZnTe), α-HgI₂ and TlBr have been developed intensely. However, each of these compounds has suffered from persistent unsolved issues related to either crystal growth or device operation.

Halide perovskites have attracted a lot of interest in the fields of photoelectrical conversion, such as photovoltaic applications, photo detection and photoemission. The structures of the halide perovskites are very diverse and form a large family, depending on various anions and cations. Among these, the all-inorganic perovskite CsPbBr₃, with a relatively large bandgap of 2.25 eV, has been proved to be feasible for growth to a large size from its melt, and also from solutions. The strong coupling between cation lone-pair Pb s orbitals and anion p orbitals results in a unique electronic band structure, resulting in an extraordinarily dispersive band structure for both conduction and valence bands.

SUMMARY

Photodetectors for detecting incident radiation, such as incident gamma-rays and incident nuclear radiation, are provided.

One embodiment of a photodetector includes: single-crystalline CsPbX₃, where X represents Br or Cl; at least one metal anode in electrical communication with the CsPbX₃, wherein the metal of the metal anode is selected from the group consisting of gallium, chromium, titanium, indium, indium-calcium alloys, lead, aluminum, magnesium and alloys of two or more thereof; at least one metal cathode in electrical communication with the CsPbX₃, wherein the metal of the cathode is selected from gold, platinum, nickel, osmium, palladium, and alloys of two or more thereof; wherein the anode and cathode are configured to apply an electric field across the material; and a detector configured to measure a signal generated by electron-hole pairs that are formed when the material is exposed to incident gamma radiation and/or nuclear radiation.

BRIEF DESCRIPTION OF THE DRAWINGS

Illustrative embodiments of the invention will hereafter be described with reference to the accompanying drawings, wherein like numerals denote like elements.

FIG. 1 depicts an optimized temperature profile used for Bridgman growth of CsPbBr₃ single crystals, as described in the Example.

FIGS. 2A and 2B show device designs for two types of photodetectors that include CsPbBr₃ single crystals as photoactive layers.

FIGS. 3A and 3B depict the mass absorption Coefficient and attenuation length for CsI, CZT and CsPbBr₃ crystals.

FIGS. 4A and 4B show the gamma ray response from the CsPbBr₃ detectors described in the Example. The cathode and anode electrodes were Au and Ga, respectively. The thickness of the sample was 0.88 mm.

FIG. 5 shows photodetection spectra for the photodetector in the Example. Increasing the applied bias resulted in the spectra being shifted to higher channel numbers, indicating improvement in the charge collection efficiency (CCE) of the device.

FIG. 6 shows a super fine ⁵⁷Co gamma ray spectrum for the photodetector in the Example. The spectrum has an extremely low contribution from the leakage current noise. The corresponding energy resolution of this detector in terms of full width at half maximum (FWHM) was 4.3% under −150 V.

FIG. 7 shows that, over a continuous working period of 1200 s, the peak channel number and count rate for the ⁵⁷Co gamma ray spectrum for the photodetector in the Example did not shift or change, indicating polarization was absent for the newly designed device.

FIG. 8 shows the energy-calibrated spectrum obtained according to the ⁵⁷Co peak position (122 keV). A series of peaks from different radioactive isotopes was clearly resolved, such as 32 keV, 47 keV, 59.5 keV and 136 keV. The linearity (or proportionality) response of the device was quite good, as indicated in the inset in FIG. 8.

FIG. 9 lists various metal electrode materials, along with their work functions.

FIG. 10 is a table listing different doping compositions for CsPbX₃ (X=Cl, Br) compounds.

FIG. 11A. Optical performance dependence on the impurities levels inside a CsPbBr₃ crystals. FIGS. 11B and 11C. Detection performance dependence on the impurities levels inside a CsPbBr₃ crystals. The detectors were with Ga and Au electrodes.

FIG. 12A-12C. Zone refining of CsPbBr₃ through a three-zone furnace. The detector performance under ⁵⁷Co γ-ray spectra obtained by CsPbBr₃ detectors fabricated from an ingot after zone refining with a 0.002 mm/s translation speed (FIG. 12A) and after subsequent Bridgman growth (FIG. 12B). The detectors were fabricated with Ga and Au electrodes (Type I). FIG. 12C. The detector performance under ⁵⁷Co γ-ray spectra obtained by CsPbBr₃ detectors fabricated from the ingot after zone refining and subsequent Bridgman growth. The Bridgman growth parameters were the same for the crystals FIG. 12B and FIG. 12C.

FIG. 13A is a schematic diagram of a detector that is encapsulated in wax. FIG. 13B shows the detector performance after encapsulation with wax in air with RH % of 50-70% over a period of 8 months. Note that the slightly increase in peak channel number (8 months later) results from the slight fine-gain increase of the amplifier.

DETAILED DESCRIPTION

Materials, photodetectors, and methods for detecting incident radiation, such as incident gamma-rays and incident nuclear radiation, are provided. Embodiments of the methods and photodetectors allow for high spectroscopic resolution of the gamma-rays from radioactive elements and X-ray sources. For example, embodiments of the methods and photodetectors are able to provide spectroscopic resolution (energy resolution) of 6% or better at a specific energy of 122 KeV, in terms of full width at half maximum (FWHM), as illustrated in the Example. This includes methods and photodetectors that provide spectroscopic resolutions of 5% or better, and methods and photodetectors that provide spectroscopic resolutions of 4.5% or better, at a specific energy of 122 KeV, in terms of FWHM.

Some embodiments of the inventions described herein are based, at least in part, on the inventors' discovery that certain anode/cathode pairs can be used with the photoactive materials in the photodetectors to provide significantly improved device performance.

One embodiment of a photodetector comprises: a material comprising a photoactive, single-crystalline semiconductor; a metal anode in electrical communication with the material; a metal cathode in electrical communication with the material, wherein the anode and cathode are configured to apply an electric field across the material; and a detector configured to measure a signal generated by electron-hole pairs that are formed when the material is exposed to incident gamma radiation and/or nuclear radiation. By way of illustration only, one such photodetector comprises a gallium anode, a gold cathode, and a CsPbBr₃ photoactive layer.

One embodiment of a method for the detection of incident radiation using a photodetector, such as that described immediately above, comprises the steps of: exposing the photoactive, single-crystalline semiconductor to incident radiation, wherein the material absorbs the incident gamma radiation and/or nuclear radiation and electron-hole pairs are generated in the material; and measuring at least one of the energy or intensity of the absorbed incident radiation by detecting the generated electrons and/or holes. During the operation of the photodetector, an electrical voltage is applied to the cathode, which collects the signal, and the anode is grounded. Or, during the operation of the photodetector, the electrical voltage is applied to the anode, which collects the signal, and the cathode is grounded.

A variety of photoactive semiconductors can be used, wherein the term photoactive semiconductor refers to a semiconductor material that absorbs gamma radiation or nuclear radiation and generates a photocurrent.

The photoactive semiconductor may be an all-inorganic semiconductor or an organic-inorganic semiconductor. For example, the photoactive semiconductor can be a photoactive perovskite, such as a halide perovskite having the formula AMX₃, where A is a monovalent alkylammonium cation (for example, methylammonium, formamidinium, or a combination thereof) or an alkali metal cation (Group I cation), X is a halide ion, and M is an octahedrally coordinated bivalent metal atom. Examples of all-inorganic perovskites include compounds such as CsPbBr₃, CsPbCl₃, RbPbBr₃, and RbPbCl₃. Examples of hybrid organic-inorganic perovskites include compounds such as APbBr₃ and APbI₃, wherein A is methylammonium and/or formamidinium.

Other suitable halide perovskites have the formula amAMX₃, where am is an alkyl diamine cation, an aromatic diamine cation, an aromatic azole cation, or a cyclic alkyl diamine cation. A is a monovalent alkylammonium cation or an alkali metal cation (Group I cation), X is a halide ion, and M is an octahedrally coordinated bivalent metal atom. The diamines can be primary, secondary, or tertiary diamines. Am can also represent a hydrazinediium cation. In some embodiments, am is an alkyl amine-functionalized aromatic azole, such as a histamine. In some embodiments, am is ethylenediamine, en. In these embodiments, the halide perovskites can be represented by the formula enAMX₃, wherein en is the ethylenediamine cation. In some embodiments, the am cation is an alkylene diammonium cation.

Other suitable inorganic semiconductor compounds have the formula AB₂X₅, where A represents Tl or In, B represents Sn or Pb, and X represents Br or I. The formula AB₂X₅ covers solid solutions that include both A elements, both B elements, and/or both X elements, as well as the end members of the formula. For the solid solutions, the formula can be written as (Tl, In)(Sn, Pb)₂(I, Br)₅. Thus, the formula covers the compounds TlSn₂I₅, InSn₂I₅, TlSn₂Br₅, TlPb₂I₅, TlPb₂Br₅, InSn₂Br₅, InPb₂I₅, and InPb₂Br₅, as well as the solid solutions Tl_(1-x)In_(x)Sn_(2-y)Pb_(y)I_(5-z)Br_(z), In_(1-x)Tl_(x)Sn_(2-y)Pb_(y)I_(5-z)Br_(z), Tl_(1-x)In_(x)Sn_(2-y)Pb_(y)Br_(5-z)I_(z), Tl_(1-x)In_(x)Pb_(2-y)Sn_(y)I_(5-z)Br_(z), Tl_(1-x)In_(x)Pb_(2-y)Sn_(y)Br_(5-z)I_(z), In_(1-x)Tl_(x)Sn_(2-y)Pb_(y)Br_(5-z)I_(z), In_(1-x)Tl_(x)Pb_(2-y)Sn_(y)I_(5-z)Br_(z), and In_(1-x)Tl_(x)Pb_(2-y)Sn_(y)Br_(5-z)I_(z), where 0≤x≤0.5; 0≤y≤1; and 0≤x≤0.2.5, and at least one of x, y, and z is greater than 0.

Still other suitable inorganic semiconductor compounds have the formula Hg₃Q₂X₂, where Q represents a chalcogen atom or a combination of chalcogen atoms (e.g., a combination of S, Se, and Te), and X represents a halogen atom or a combination of halogen atoms. Still other suitable inorganic semiconductor compounds include chalcohalides. For example, chalcogenides having the chemical formula A₆BX₄, wherein A is a metal, B is sulfur or selenium, and X is a halide can be used as the photoactive semiconductor. Members of this class of chalcohalides include thallium-based chalcohalides, such as Tl₆SI₄, Tl₆SBr₄ and Tl₆SeI₄. Still other suitable inorganic compounds have the formula A₂P₂X₆, where A represents Pb or Sn and X represents S or Se. Still other photoactive semiconductors include copper halide chalcogenides, such as Cu₂I₂Se₆ and its solid solutions, which include other halogens and/or other chalcogens. Examples of these have the formulas Cu₂I_(x)Br_(2-x)Se_(y)Te_(6-y) and Cu₂I_(x)Br_(2-x)Se_(y)S_(6-y), where 0≤x≤1 and 0≤y≤3.

Various members of the aforementioned photoactive semiconductors, as well as other suitable photoactive semiconductors, can be categorized as inorganic compounds comprising at least three elements, wherein at least one of the three elements is an element from period five or period six of the Periodic Table of the Elements and another of the three elements is selected from S, Se, Te, CI, F, I and Br. This category of semiconductors includes: AB₂Q₄ compounds with A=Cd, Hg or Pb; B=AI, Ga, or In; and Q=S, Se, or Te; TIBQ₂ compounds with B=AI, Ga, or In; and Q=S, Se, or Te; (A₂Q)_(m)(AX)n with A=Na, K, Rb, Cs or TI; Q=S, Se, or Te; and X=F, CI, Br or I; (AX)_(m)(BX₂)_(n) with A=Na, K, Rb, Cs or Tl; B=Cu, Zn, Cd, or Hg; and X=F, CI, Br or I; (Pn₂Q₃)_(m)(PnX₃)_(n) with Pn=N, P, As, Sb or Bi; Q=S, Se, or Te; and X=F, CI, Br or I; (A₂Q)_(m)(Au₂Q)_(n) with A=Na, K, Rb, Cs or TI; and Q=S, Se, or Te; (A₂Q)_(m)(BQ)_(n) with A=Na, K, Rb, Cs or Tl; B=Cd or Hg; and Q=S, Se or Te; (Tl₂S)_(m)(SnS₂)_(n); and (A₂Q)_(m)(Pn₂Q₃)_(n) with A=Na, K, Rb, Cs or TI; Pn=P, As, Sb, or Bi; and Q=S, Se, or Te.

A description of photoactive semiconductors and methods of making them can be found in U.S. Pat. No. 8,519,347 and PCT patent application publication number No. WO2017030624, the disclosures of which are incorporated herein by reference.

Examples of metals that can be used as anodes for a photoactive layer of CsPbBr₃ include gallium, chromium, titanium, indium and alloys thereof. Examples of metals that can be used as cathodes for a photoactive layer of CsPbBr₃ include gold, platinum, nickel, osmium and palladium, and alloys thereof.

EXAMPLES Example 1

In this example, a modified melt growth method was deployed for the improved crystal growth of CsPbBr₃ and CsPbCl₃. The resistivity of CsPbBr₃ is on the order of 10⁹-10¹⁰ Ω·cm, depending on the purity level. This example demonstrates a new, effective device and method of collection that has been developed. CsPbBr₃ detectors with new designs were demonstrated to have clearly resolved the 59.5 keV ²⁴¹Am gamma ray spectrum and 122 KeV ⁵⁷Co spectrum, with a specific μτ of >1×10⁻³ cm²/V, which is comparable to benchmark CdZnTe and CdTe crystals. A super-fine spectrum for a different radiative isotope was also analyzed for the first time, with energy resolution of 4.3% for a ⁵⁷Co gamma ray with a specific energy of 122 KeV.

Crystal Growth of CsPbBr₃

Obtaining a high-quality, single crystal of CsPbBr₃ was difficult due to the phase transition occurring at a relatively low temperature (<150° C.). The first phase transition from cubic (Pm-3m) to tetragonal (P4/mbm) was a first-order phase transition, accompanied by volume and enthalpy changes with respect to temperature. Such discontinuous derivations during the phase transition-induced residual stress or mechanical deformations, which enhanced the initiation and propagation of cracks, sub-grain boundaries, or twins. Such structural defects behave like recombination or trapping centers and are detrimental to the detector performance, and thus should be prevented during crystal growth.

The kinetic parameters for the crystal growth processes are extremely important to obtaining a high-quality, single-crystal ingot. The overheating temperature, temperature gradient, in-situ annealing, and cooling strategy were evaluated carefully and tested accordingly. Dramatic improvements were achieved through the optimized, controlled crystal growth processes described here. The optimized temperature profile used for vertical Bridgman growth is indicated in FIG. 1, including a specific overheating temperature of 15 K, and a temperature gradient of 9 K/cm, due to the intrinsic thermal conductivity of CsPbBr₃ being quite small. Therefore, a smaller translation speed was desired for Bridgman growth. The single-crystal ingot was grown with a dropping velocity of 0.5 mm/h. The cooling strategy was also very important because of the low-temperature phase transition. The cooling rate used here was ˜5 K/h, and a single-crystal ingot with a diameter of 11 mm and a length of 7 cm was obtained. The orange-red single crystal ingot was translucent and free of cracks or grain boundaries. The ingot was then cut and fabricated into different wafers with regular shapes. Owing to the relatively weak mechanical properties and cleavage characteristic of CsPbBr₃, the wafers were handled with great care to avoid chipping or cracks.

Crystal Growth of CsPbCl₃

CsPbCl₃ was synthesized directly by combining equal amount of CsCl and PbCl₂ through solid-state reaction. After synthesis, vertical Bridgman melt growth was employed to grow large single crystals. The silica crucible for Bridgman melt growth had a tapered shape and 11 mm inner diameter. It should be noted that the silica tube was flame-sealed with a residual pressure below 10⁻⁴ Torr. During Bridgman growth, the translation system is constructed to achieve very small but constant dropping velocity, in the range of 0.1˜1 mm/h. The overheating temperature is set to 620° C. for 10 h. Once the quartz tube has completely passed through the temperature gradient region, the ingot was subsequently cooled down to room temperature in 20 h.

Device Design for CsPbBr₃ Devices

A new electrode configuration design for the CsPbBr₃ detectors was applied. The as-grown intrinsic CsPbBr₃ single crystal was shown to be a p type material, owing to its positive Seebeck coefficient at room temperature. Thus, the fermi level of CsPbBr₃ should have been close to the valence band. An energy level diagram of the conduction and valence bands of CsPbBr₃ is provided in Liang, J., et al., All-Inorganic Perovskite Solar Cells. J. Am. Chem. Soc. 2016, 138 (49), 15829-15832.

As illustrated, there are two basic types (type I and type II) of planar devices for CsPbBr₃ (FIGS. 2A and 2B). For the type II design, the metals with high work functions are usually Au, Pt and Pd. With the type II design, the corresponding energy diagram under high bias is described in FIG. 3B. Owing to its small Schottky barrier, the hole can be easily injected into the crystal from the positive electrode through tunneling or a thermionic emission mechanism, which contributes to a large leakage current (FIG. 4B). For such a device, the leakage current is not stable over time, and usually increases continuously over time. Therefore, the planar device with the type II design cannot behave as a gamma ray detector. The resulting background noise from the leakage current of the detector dominates the spectrum.

A new electrode design, as indicated in FIG. 2A, has been proposed here. A metal with a relatively low work function was utilized as an anode, while a metal with a relatively high work function served as the cathode. The high electrical voltage and signal collection were all from the cathode. The anode was grounded during detection. This design took into consideration the experimental p type character of CsPbBr₃. The energy diagram for this system has large Schottky barriers for both the electron and the hole at the semiconductor-metal interface while the device was biased, as shown is FIG. 3A. For this device, the I-V characteristic curve was not linear, but rather was like a diode. Under the negative side (FIG. 4A), the leakage current was quite small, around 15 nA, and under 200 V (corresponding to ˜250 V/mm). The leakage was also very stable over time. While reserving the bias (FIG. 4A, positive side), the leakage current increased dramatically owing to the injection from both positive and negative electrodes.

Poly[bis(4-phenyl)(2,5,6-trimethylphenyl)amine (PTAA) was used as a hole transport layer materials for better hole collection. The use of PTAA increased the Schottky barrier slightly; however, it did not change the energy resolved spectrum significantly.

The electrode configuration based on the above new design concept is not confined to planar-type detectors; it can also be applied to other type of detectors, such as co-planar detectors, pixel detectors and hemisphere type detectors.

Device Characterization

CsPbBr₃ is a high Z compound with an effective atomic number of 65.9, which is much higher than CdTe (50.2) and comparable to HgI₂ (68.9). The cross-section for photoelectric absorption in a material of atomic number Z varies as Z^(n). Therefore, the higher atomic number promises higher stopping power for X and gamma ray photons. The attenuation coefficients of CsPbBr₃ are higher than those of CZT, especially in the high energy region. For instance, for ⁵⁷Co y-rays with characteristic energy of 122 keV, the attenuation lengths are 1.70 mm for CdTe/CZT, and 1.20 mm for CsPbBr₃, confirming the higher stopping power for high-energy photons. Therefore, thinner crystals can be used to absorb hard radiation with the same energy.

Under the ²⁴¹Am gamma source (59.5 keV), the CsPbBr₃ device showed a well resolved spectroscopic spectrum. Owing to the intensity of the ²⁴¹Am gamma source, the accumulation time was usually longer than the ⁵⁷Co gamma ray source. During the measurement, the Ga anode was under irradiation; thus, the measured signal was generated mainly by hole drift through the thickness of device. The spectra also indicated the distinct transport properties of the electron and the hole. While increasing the applied bias, the spectra shifted to the higher channel number (FIG. 5), indicating an improvement in the charge collection efficiency (CCE). A super fine ⁵⁷Co gamma ray spectrum with extremely low contribution from the leakage current noise is indicated in FIG. 6, and the corresponding energy resolution of this detector in terms of full width at half maximum (FWHM) was 4.3% under −150 V.

The device also showed very stable response with time. Over a continuous working period of 1200 s, the peak channel number and count rate for the ⁵⁷Co gamma ray spectrum did not shift or change (FIG. 7), indicating polarization was absent for the newly designed device.

The energy-calibrated spectrum (FIG. 8) was also obtained according to the ⁵⁷Co peak position (122 keV). A series of peaks from different radioactive isotopes was clearly resolved, such as 32 keV, 47 keV, 59.5 keV and 136 keV. The linearity (or proportionality) response of the device was quite good, as indicated in the inset in FIG. 8. This was very important for the application of radioactive isotope classification.

The mobility-lifetime product evaluated here for the hole and electron were 1.34×10⁻³ and 8.77×10⁻⁴ cm²/V, respectively, according to the Hecht equation. (See, e.g., He, Y., et al., Defect Antiperovskite Compounds Hg₃Q₂I₂ (Q=S, Se, and Te) for Room-Temperature Hard Radiation Detection. J. Am. Chem. Soc. 2017, 139 (23), 7939-7951.) The transport property was much better for the hole, which is quite unique among the materials in this field. The mobility-lifetime product values for CsPbBr₃ were found to be comparable to those of the benchmark CdTe and CZT materials when determined using the same method.

The carrier drift mobilities of the crystals were evaluated using the rise time t_(r) of transient waveforms from the preamplifier under a ²⁴¹Am gamma ray source. (See, e.g., Sellin, P. J., et al., Drift mobility and mobility-lifetime products in CdTe:Cl grown by the travelling heater method. IEEE Trans. Nucl. Sci. 2005, 52 (6), 3074-3078; and Szeles, C., CdZnTe and CdTe materials for X-ray and gamma ray radiation detector applications. physica status solidi (b) 2004, 241 (3), 783-790.) For photo-generated carriers drifting across the thickness, the mobility μ was given

${= \frac{d^{2}}{U\; t_{r}}},$ where U is the applied bias across the thickness d, and t_(r) is the transit time of the carriers through the device. The electron and hole mobility values obtained were 363 and 52 cm²/(V·s), respectively.

A similar spectroscopic response has been reproducibly obtained from different batches of materials. The robustness and reproducibility of the new device design have improved the CsPbBr₃ to the level of the ideal room temperature radiation detector, with a low cost, an ability to easily scale up, and high performance.

Experimental Section

Materials. Chemicals in this work were used as obtained, including: (i) Cesium bromide, 99.999%, Sigma-Aldrich; (ii) Lead bromide, 99.999%, Sigma-Aldrich.

Bridgman growth of CsPbBr₃ from its melt. Polycrystalline CsPbBr₃ was prepared directly from CsBr and PbBr₂ by solid-state reaction. For a small-amount (<40 g) Bridgman growth run, the synthesis and growth was usually done in the same quartz tube to reduce the unintended impurity contamination from multi-step operations. The tube for such growth had a tapered shape and a Φ13 mm diameter. For a large-amount (>100 g) Bridgman growth run, the synthesis and growth processes were done separately. First, the polycrystalline CsPbBr₃ was further purified by fast Bridgman runs. Then only the middle part of the polycrystalline ingot was used for the following growth. The tube for such Bridgman growth also had a tapered shape and a Φ25 mm diameter. All the reactions for synthesis and crystal growth were done in a vacuum, with an original pressure less than 10⁻⁴ Torr (at room temperature). Any moisture contamination of the starting materials and ternary compound was likely to lead to lead oxide and off-stoichiometric issues. The quartz tube was then placed on a support rod which moved downwards with a geared dropping system in a two-zone vertical furnace. This translation system was constructed to achieve a very small but constant dropping velocity, in the range of 0.1˜1 mm/h. For the Bridgman growth, the quartz tube was heated up to 580° C. in 10 h and held at that temperature for 12 h. In practice, 20˜30 K superheating helps to reduce the excess nucleation centers and suppress the possibility of the formation of structural defects. The temperature profile (FIG. 1) for the Bridgman growth was also optimized to avoid any thermal-induced cracks and possible constitutional super-cooling, and to enhance the single crystal yield of the CsPbBr₃. The measured temperature gradient in FIG. 1 was about 9 K/cm. Once the quartz tube had been completely passed through the temperature gradient region, the ingot was then cooled down to 200° C. in 20 h subsequently. Owing to the existence of phase transitions, the ingot was then cooled down to room temperature with a very slow cooling rate of 2˜5 K/h.

Mechanical Processing and Polishing. The CsPbBr₃ crystal ingots were cut into rounded wafers perpendicular to the growth direction or desired shapes of 0.5˜2 mm thickness using a Struers Accutom-50 waferizing saw equipped with a 300 μm wide diamond-impregnated blade. The sample surface was polished mechanically with successively fine SiC grinding papers down to a 1 μm particle size. Owing to the low hardness of CsPbBr₃, the pressing pressure during mechanical polishing was kept low enough to avoid inducing post-growth structural defects.

Electrode preparation. The as-polished CsPbBr₃ crystals were rinsed in acetone to remove the possible surface contamination before the electrode deposition. Two methods were used to prepare the Au electrode: brushing Au paint, and thermal evaporation through a shielding mask onto CsPbBr₃ samples. The Ga electrode was prepared simply by brushing liquid Ga metal onto the surface of the crystal. The electrodes were then connected by a Cu wire to the outer collection circuit. An Al electrode (low work function metal) deposited by thermal evaporation was also tried; however, the Al contact was not stable in air and tended to peel off quickly upon exposure to air. Therefore, the contact had to be encapsulated to protect it from exposure to air. Other low and high work function metals are listed in FIG. 9.

Electrical Properties and Detector Performance Measurements. The I-V characteristic curves were measured in the dark using a Keithley 6517B electrometer. The resistivity was then calculated from the I-V characteristics in the low bias range.

For detector performance measurements, the gamma ray sources employed were ²⁴¹Am 59.5 KeV, 0.2 mCi ⁵⁷Co 122 KeV, and 5 μCi ¹³⁷Cs 662 KeV γ-ray sources. In each measurement, the as-prepared detectors were enclosed in a shielding box connected to an eV-550 preamplifier. A negative bias varying from −4 to −300 V was applied to the bottom contact, while the γ-ray source was irradiated from the top cathode contact. The signals from the preamplifier were further amplified and shaped by the ORTEC amplifier (Model 572A) with a gain of 100-500 and a shaping time of 1-10 μs. The final signals were subsequently evaluated by a dual 16 K input multichannel analyzer (Model ASPEC-927) and read into the MAESTRO-32 software, which generated and displayed the response spectrum. The mobility was estimated using pulse height spectroscopy. For the mobility evaluation, signals from the preamplifier, instead of transferring to the ORTEC amplifier, were collected by using a homemade interface based on National Instruments software, which could capture the complete transient waveforms directly from the preamplifier with a maximum time resolution of 4 ns. Each transient waveform was analyzed to determine its rise time t_(r), which corresponded to a transit time between 10% and 90% of the amplitude of the transient pulses.

Example 2

This example illustrates that the electrical and detector performance of CsPbBr₃ and CsPbCl₃ can be modified through intentionally doping. Doping can take place done during the Bridgman growth from a melt or during solution-phase growth. The doping elements can be selected from elements of the chemical periodic table having atomic numbers, Z, in the range from 1 to 83, including elements or compounds from Group 13 to Group 17 of the periodic table of the elements.

Bridgman growth of Doped CsPbBr₃ (CsPbBr₃:Dopant) from its melt. The binary compounds CsBr, PbBr₂ and TlBr were used to synthesize the Tl-doped polycrystalline CsPbBr₃ by a solid-state reaction. The chemical ratio for CsBr and PbBr₂ was 1:1, while TlBr was added with a ratio of 0.05%-0.5% (atomic %; at. %). The temperature for the synthesis was set at 580° C. After synthesis, the Tl-doped polycrystalline CsPbBr₃ was used for Bridgman growth. The silica tube for Bridgman growth was of 11 mm inner diameter with a conically shaped end. All processes for synthesis and crystal growth were done in vacuum, with an original pressure of less than 10⁻⁴ Torr (at room temperature). The Bridgman growth procedure for Tl-doped CsPbBr₃ was the same as that for the non-doped CsPbBr₃. The silica tube was heated to 590° C. in 10 h and held at that temperature for 12 h for overheating (15-30 K) to avoid heterogeneous nucleation. Once the silica tube completely passed, with a dropping speed of 0.5 to 2 mm h⁻¹, through the temperature gradient region (with a typical temperature gradient of 5 to 20 K cm⁻¹), the resulting ingot was cooled down to 200° C. in 20 h. The ingot was then cooled down to room temperature with a cooling rate of 2 to 5 K h⁻¹.

The resistivity of as-grown crystals (YH2088) was over 10⁹ Ω·cm, which is at least one order of magnitude higher than intrinsic CsPbBr₃ crystals.

Doping with elements other than Tl can be carried out using the same general procedure. The Table in FIG. 10 lists other possible dopant elements, along with illustrative concentration (in at. %) that can be used. As shown in the table of FIG. 10, the crystals were doped with other dopants (e.g., Te (0.5% at. %), Bi (0.2% at. %), TlBr (0.5% at. %), PbCl₂ (5% at. %), Se (0.2% at. %), PbCl₂ (0.5% at. %), PbCl₂ (1% at. %), PbCl₂ (5% at. %), In (0.2% at. %), Ga (0.2% at. %), Sb (0.2% at. %), Pb and PbBr₂ (1% at. % for Pb and 1% at. % for PbBr₂)). Through such doping, the crystals demonstrated high resistivities of at least 10⁹ Ω·cm.

For example, additional Pb metal can be introduced as a dopant into the stochiometric ternary compound for the purpose of defect compensation (see sample YH2010 in FIG. 10). The Pb-doped CsPbBr₃ detector showed comparable or higher detector performance relative to the detector made from the non-intentionally doped crystals; achieving ˜5% energy resolution under 122 keV ⁵⁷Co γ ray.

In addition, iodine (I) doping of CsPbBr₃ single crystal (YH2015, 0.1% at. % PbI₂) was performed. Upon exposure to a ⁵⁷Co γ-ray source, the I-doped CsPbBr₃ detector with Ga and Au electrodes also delivered a series of excellent ⁵⁷Co γ-ray spectra with extremely low contributions from leakage current noise and achieved an energy resolution of 5.3% under −350 V.

Pure CsPbCl₃ and Br-doped CsPbCl₃ single crystals were also grown using the Bridgman method, as indicated in the table of FIG. 10. The measured electrical resistivity for the pure CsPbCl₃ single crystal was at least ˜1.7×10⁹ Ω·cm. Based on the bias-dependent channel number of the γ-ray peaks, the (μτ)_(h) calculated according to the Hecht equation is at least 3.2×10⁻⁴ cm²/V. The energy resolution achieved by the pure CsPbCl₃ with Ga and Au contacts was ˜16% for 122 keV ⁵⁷Co γ ray.

Zone-refining for purification. Crystals grown with different purity levels showed distinct electrical and, thus, detection properties (FIGS. 11A-11C). The “high purity” sample contained less than 10 ppm total impurities according to a glow discharge mass spectrometry (GDMS) analysis, while the “low purity” sample contained more than 30 ppm impurities. The higher impurity level reduced transmission level of the incident light with wavelength over 570 nm from >60% to ˜30% (FIG. 11A), which was also confirmed by a color change of the crystals. A detector made from the “low purity” sample demonstrated much worse detector performance than that made from the “high purity” sample, as shown in FIGS. 11B and 11C. The hole mobility-lifetime product for “low purity” and “high purity” samples were <10⁻⁴ cm²/(Vs) and >10⁻³ cm²/(Vs), respectively.

To purify and further improve the crystal quality, a three-zone horizontal zone-refining furnace was used. As an example, the temperature for each zone can be set to be identical in the range of 600-650° C., the translation speed was 0.001 to 0.1 mm/s. Once the entire crucible containing CsPbBr₃ or CsPbCl₃ was passed through the three zones, the crucible was moved to the starting point in 10 s to start another pass-through. Thus, one pass implies the ingot had been directionally melted and solidified three times owing to the three heating zones. After zone-refining, impurities accumulated in a black part at the last-freezing part of the ingot along the zone-refining direction. The black end was removed and the remaining clear part was used for the subsequent Bridgman growth.

After the zone-refining, Bridgman growth was conducted. The detector performance is shown in FIGS. 12A, 12B, and 12C. The purity for the starting materials for the sample in FIGS. 12A-12C were 5N for CsBr and 4N8 for PbBr₂. The detector made from the clear part after zone-refining showed distinct gamma ray response from the background. Bridgman growth resulting in a detector that demonstrated excellent detector performance (FIG. 12B).

The same procedure was carried out on starting materials with lower purities (No. YH2081, 3N for CsBr and 4N8 for PbBr₂); however, after 10 passes and Bridgman growth (same to YH2090B), the detector made from the sample YH2081 ingot did not have a high gamma ray response, as demonstrated in FIG. 12 C, demonstrating that the impurity levels inside the single crystals of CsPbBr₃ and CsPbCl₃ played an important role in determining the detector performance. At least over 4N or higher purify level was required to achieve the highest detector performance in this illustrative example, in terms of producing a resolved peak under gamma ray exposure and possessing a high mobility-lifetime product >10⁻⁴ cm²/(Vs).

Encapsulation of CsPbBr₃ and CsPbCl₃ detector for long-term use. A CsPbBr₃ single crystal can be stable under atmospheric conditions for years. However, they will decompose into binaries in contact with water. Thus, the CsPbBr₃ device might decompose in humid conditions. The initial energy resolution of a CsPbBr₃ detector with Ga and Au contacts under a relative humidity (RH) of 60-70% degraded from ˜5% to over 10% in 2 weeks. After encapsulation with wax, the CsPbBr₃ detector was stable for over 8 months, with a negligible change in energy resolution (˜5-6%), as indicated in FIG. 13B. The encapsulated detector (FIG. 13A) also showed stable electrical properties over time. The dark current was also unchanged with time. Thus, encapsulation of a CsPbBr₃ detector to protect it from exposure to air and water can be used to achieve long-term stability of the detector performance. Polydimethylsiloxane (PDMS) is another suitable encapsulant.

The word “illustrative” is used herein to mean serving as an example, instance, or illustration. Any aspect or design described herein as “illustrative” is not necessarily to be construed as preferred or advantageous over other aspects or designs. Still further, the use of “and” or “or” is intended to include “and/or” unless specifically indicated otherwise.

The foregoing description of illustrative embodiments of the invention has been presented for purposes of illustration and of description. It is not intended to be exhaustive or to limit the invention to the precise form disclosed, and modifications and variations are possible in light of the above teachings or may be acquired from practice of the invention. The embodiments were chosen and described in order to explain the principles of the invention and as practical applications of the invention to enable one skilled in the art to utilize the invention in various embodiments and with various modifications as suited to the particular use contemplated. It is intended that the scope of the invention be defined by the claims appended hereto and their equivalents. 

What is claimed is:
 1. A device for the detection of incident radiation comprising: single-crystalline CsPbX₃, where X represents Br or Cl; at least one metal anode in electrical communication with the CsPbX₃; at least one metal cathode in electrical communication with the CsPbX₃, wherein the metal anode is selected from the group consisting of a gallium anode, an indium anode, an aluminum anode, a lead anode, and a magnesium anode, and the metal cathode is selected from a gold cathode and a platinum cathode; a detector configured to measure a signal generated by electron-hole pairs that are formed when the material is exposed to incident gamma radiation and/or nuclear radiation.
 2. The device of claim 1, wherein the metal anode is the gallium anode.
 3. The device of claim 2, wherein the metal cathode is the gold cathode.
 4. The device of claim 3, wherein X represents Br and the metal cathode is the gold cathode.
 5. The device of claim 2, wherein the metal cathode is the platinum cathode.
 6. The device of claim 1, wherein the metal anode is the indium anode.
 7. The device of claim 6, wherein the metal cathode is the gold cathode.
 8. The device of claim 6, wherein the metal cathode is the platinum cathode.
 9. The device of claim 1, wherein the metal anode is the aluminum anode.
 10. The device of claim 9, wherein the metal cathode is the gold cathode.
 11. The device of claim 9, wherein the metal cathode is the platinum cathode.
 12. The device of claim 1, wherein the metal anode is the lead anode.
 13. The device of claim 12, wherein the metal cathode is the gold cathode.
 14. The device of claim 12, wherein the metal cathode is the platinum cathode.
 15. The device of claim 1, wherein the metal anode is the magnesium anode.
 16. The device of claim 15, wherein the metal cathode is a gold cathode.
 17. The device of claim 15, wherein the metal cathode is the platinum cathode.
 18. The device of claim 1, wherein the CsPbX₃ is intentionally doped with an element having an atomic number in the range from 1 to
 83. 19. The device of claim 18, wherein the CsPbX₃ has a purity of at least 99.99%, excluding the intentional dopants.
 20. The device of claim 1, wherein the device is encapsulated in wax or a polymer coating.
 21. A method for detecting incident radiation using a device for comprising: single-crystalline CsPbX₃, where X represents Br or Cl; at least one metal anode in electrical communication with the CsPbX₃; at least one metal cathode in electrical communication with the CsPbX₃, wherein the metal anode is selected from the group consisting of a gallium anode, an indium anode, an aluminum anode, a lead anode, and a magnesium anode, and the metal cathode is selected from a gold cathode and a platinum cathode; a detector configured to measure a signal generated by electron-hole pairs that are formed when the material is exposed to incident gamma radiation and/or nuclear radiation, the method comprising: exposing the photoactive, single-crystalline semiconductor to incident gamma radiation and/or nuclear radiation, wherein the material absorbs the incident gamma radiation and/or nuclear radiation and electron-hole pairs are generated in the material; and measuring at least one of the energy or intensity of the absorbed incident gamma radiation by detecting the generated electrons, holes, or both. 